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physics.space-ph2026

Evolution and Impact of Switchbacks Throughout the Heliosphere

Alfred Mallet, Chen Shi, Anna Tenerani +23

Magnetic switchbacks are large-amplitude fluctuations in the interplanetary magnetic field, and appear frequently in the near-Sun solar wind explored recently by Parker Solar Probe…

physics.space-ph2026

Properties of Magnetic Switchbacks in the Near-Sun Solar Wind

Samuel T. Badman, Naïs Fargette, Lorenzo Matteini +24

Magnetic switchbacks are fluctuations in the solar wind in which the interplanetary magnetic field sharply deflects away from its background direction so as to create folds in magn…

physics.space-ph2025

The Temperature Anisotropy and Helium Abundance Features of Alfvénic Slow Solar Wind Observed by Parker Solar Probe, Helios, and Wind Missions

Jia Huang, Davin E. Larson, Tamar Ervin +20

Slow solar wind is typically characterized as having low Alfvénicity, but the occasional occurrence of highly Alfvénic slow solar wind (HASSW) raises questions about its source r…

physics.space-ph2025

The evolution of CME sheath turbulence from L1 to Earth: Wind and MMS observations of the 2023-04-23 CME

Matthew R. Argall, Li-Jen Chen, Noé Lugaz +5

An interplanetary shock driven by a coronal mass ejection (CME) containing an interval of sub-Alfvénic flow impacted Earth on April 23, 2024. In this article, we analyze the turbu…

physics.space-ph2024

Acceleration of electrons and ions by an "almost" astrophysical shock in the heliosphere

Immanuel Christopher Jebaraj, Oleksiy Agapitov, Vladimir Krasnoselskikh +18

Collisionless shock waves, ubiquitous in the universe, are crucial for particle acceleration in various astrophysical systems. Currently, the heliosphere is the only natural enviro…